Diffuse gamma-ray emission from galactic pulsars

Understand

Millisecond Pulsars are second most abundant source population discovered by the Fermi-LAT.

• They might contribute non-negligibly to the diffuse emission measured at high latitudes by Fermi-LAT, the IDGRB.
• Gamma-ray sources also contribute to the anisotropy of the IDGRB measured on small scales by Fermi-LAT.
• We aim to assess the contribution of the unresolved counterpart of the detected MSPs population to the IDGRB and the maximal fraction of the measured anisotropy produced by this source class.